HR 8832
Observation data Epoch J2000 Equinox J2000 |
|
---|---|
Constellation | Cassiopeia |
Right ascension | 23h 13m 16.97632s[1] |
Declination | +57° 10′ 06.0823″[1] |
Apparent magnitude (V) | 5.574[2] |
Characteristics | |
Spectral type | K3 V[3] |
U−B color index | +0.902[2] |
B−V color index | +0.983[2] |
Variable type | Suspected[4] |
Astrometry | |
Radial velocity (Rv) | –18.5[5] km/s |
Proper motion (μ) | RA: +2075.07±0.33[1] mas/yr Dec.: +295.45±0.25[1] mas/yr |
Parallax (π) | 152.76 ± 0.29[1] mas |
Distance | 21.35 ± 0.04 ly (6.55 ± 0.01 pc) |
Absolute magnitude (MV) | 6.50 |
Details | |
Mass | 0.794+0.037 −0.022[6] M☉ |
Radius | 0.80±0.04[7] R☉ |
Luminosity | 0.28[note 1] L☉ |
Surface gravity (log g) | 4.50[3] cgs |
Temperature | 4710[3] K |
Metallicity [Fe/H] | +0.20[3] dex |
Rotational velocity (v sin i) | 6.94[8] km/s |
Age | ~12.46[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HR 8832 (or HD 219134, or Gliese 892) is a main sequence star in the constellation of Cassiopeia. It is smaller and less luminous than our Sun, with a spectral class of K3V, which makes it an orange-red hued star. HR 8832 is relatively close to our system, with an estimated distance of 21.25 light years. This star is close to the limit of apparent magnitude that can still be seen by the unaided eye. The limit is considered to be magnitude 6 for most observers.
This star has a magnitude 9.4 companion at an angular separation of 106.6 arcseconds.[10] The star is reported to host a rocky super-Earth, HD 219134 b, based on size (1.6 times the size of Earth), and density (6 grams per cubic cm).[11][12] A further three exoplanets, two super-Earths and one Jovian world, have been deduced using Harps-N radial velocity data.[13] Two more were discovered two months later.[14]
Planetary system
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.012±0.001 MJ | 0.038474±8e-07 | 3.0931±0.0001 | 0.0+0.13 −0.0 |
85.058±0.08° | 0.1433±0.0077 RJ |
c | 0.011±0.002 MJ | 0.064816±4e-06 | 6.7635±0.0006 | 0.0+0.26 −0.0 |
— | — |
f | 0.028±0.003 MJ | 0.14574±2e-05 | 22.805±0.005 | 0.0 | — | — |
d | 0.067±0.004 MJ | 0.23508±4e-06 | 46.71±0.01 | 0.0 | — | — |
g | 0.034±0.004 MJ | 0.3753±0.0004 | 94.2±0.2 | — | — | — |
e | 0.0117+0.19 −0.006 MJ |
2.56+3.41 −0.15 |
1842.0+4199.0 −292.0 |
0.34±0.17 | — | — |
h | 0.34 MJ | 3.11±0.04 | 2247.0±43.0 | 0.06±0.04 | — | — |
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 3.0 3.1 3.2 3.3 Lua error in package.lua at line 80: module 'strict' not found.
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- ↑ 6.0 6.1 Lua error in package.lua at line 80: module 'strict' not found.
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- ↑ http://exoplanet.eu/catalog/hd_219134_b/
- ↑ http://exoplanet.eu/catalog/hd_219134_c/
- ↑ http://exoplanet.eu/catalog/hd_219134_d/
- ↑ http://exoplanet.eu/catalog/hd_219134_e/
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
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Notes
- ↑ From , where is the luminosity, is the radius, is the effective surface temperature and is the Stefan–Boltzmann constant
External links
- Lua error in package.lua at line 80: module 'strict' not found.